中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
An unusual long-lived relativistic electron enhancement event excited by sequential CMEs

文献类型:期刊论文

作者Yang, Xiao C.; Zhu, Guang W.; Zhang, Xiao X.; Sun, Yue Q.; Liang, Jin B.; Wei, Xin H.
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2014
卷号119期号:11页码:9038-9050
关键词relativistic electron solar wind interplanetary magnetic field geomagnetic storm substorm plasmapause
ISSN号2169-9380
通讯作者Yang, XC (reprint author), Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing, Peoples R China.
英文摘要An unusual long-lived intense relativistic electron enhancement event from July to August 2004 is examined using data from Fengyun-1, POES, GOES, ACE, the Cluster Mission, and geomagnetic indices. During the initial 6days of this event, the observed fluxes in the outer zone enhanced continuously, and their maximum increased from 2.1x10(2)cm(-2)sr(-1)s(-1) to 3.5x10(4)cm(-2)sr(-1)s(-1), the region of enhanced fluxes extended from L=3.5-6.5 to L=2.5-6.5, and the flux peak location shifted inward from L4.2 to L3.3. During the following 7days, without any locational movement, the flux peak increased slowly and exceeded the prestorm fluxes by about 4 orders of magnitude. Subsequently, the decay rate of relativistic electrons is so slow that the peak remains over 10(4)cm(-2)sr(-1)s(-1) for about 30days. The drift resonance between ULF waves, which arose from high-speed solar wind and frequent impulses of solar wind dynamic pressure, and energetic electrons injected by substorms could be an important acceleration mechanism in this event. The local acceleration by whistler mode chorus could be another mechanism contributing to this enhancement. The plasmaspheric response to the interplanetary disturbances reveals that the enhanced outer zone is divided into two portions by the plasmapause. Accordingly, the slow loss rate in the plasmasphere due to hiss primarily contributed to the long-lived characteristic of this event. This event reveals that the outer zone population behaviors are dominated by the interplanetary variations together with the responses of geomagnetic field and plasmasphere to these variations.
收录类别SCI
语种英语
源URL[http://ir.nssc.ac.cn/handle/122/4381]  
专题国家空间科学中心_空间环境部
推荐引用方式
GB/T 7714
Yang, Xiao C.,Zhu, Guang W.,Zhang, Xiao X.,et al. An unusual long-lived relativistic electron enhancement event excited by sequential CMEs[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2014,119(11):9038-9050.
APA Yang, Xiao C.,Zhu, Guang W.,Zhang, Xiao X.,Sun, Yue Q.,Liang, Jin B.,&Wei, Xin H..(2014).An unusual long-lived relativistic electron enhancement event excited by sequential CMEs.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,119(11),9038-9050.
MLA Yang, Xiao C.,et al."An unusual long-lived relativistic electron enhancement event excited by sequential CMEs".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 119.11(2014):9038-9050.

入库方式: OAI收割

来源:国家空间科学中心

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。